Figure 2 from A Persistent Disk Wind in GRS 1915+105 with NICER

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A Persistent Disk Wind in GRS 1915+105 with NICER

Authors: J. Neilsen, E. Cackett, R. A. Remillard, J. Homan, J. F. Steiner, K. Gendreau, Z. Arzoumanian, G. Prigozhin, B. LaMarr, J. Doty, S. Eikenberry, F. Tombesi, R. Ludlam, E. Kara, D. Altamirano, and A. C. Fabian

2018 The Astrophysical Journal Letters 860 L19.

Provider: AAS Journals

Caption: Figure 2.

Absorption line flux (top) and equivalent width (bottom) vs. average count rate (left), 6–12 keV/2–4 keV hardness ratio (middle), and fractional rms (right) for both Fe XXVI (black filled circles) and Fe XXV (pink open circles). Non-detections are shown as 2σ upper limits.

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